We present a rigorous study of compact objects within f (Q) gravity where electrical fields
and dark matter are studied and provide novel mass–radius relations with models falling in …

We explore the presence of self-interacting bosonic dark matter (DM) within neutron stars
(NSs) in light of the latest multimessenger observations of the Neutron Star Interior …

A study on massive compact objects influenced by Bose–Einstein condensation (BEC) dark
matter (DM) with a gravitational decoupling approach is presented within the context of f (Q) …

We investigate the structure of admixed neutron stars with a regular hadronic component
and a fraction of fermionic self-interacting dark matter. Using two limiting equations of state …

We investigate the structure and the tidal deformability of the color-flavor locked strange
stars admixed with mirror dark matter. Assuming the stars in the GW170817 event have a …

Anisotropy in pressure within a star emerges from exotic internal processes. In this study, we
incorporate pressure anisotropy using the Quasi-Local model. Macroscopic properties …

Non-radial oscillations of Neutron Stars (NSs) provide a means to learn important details
regarding their interior composition and equation of state. We consider the effects of Δ …

Neutron stars (NSs) have generally been considered as cold, zero-temperature entities.
Recent progress in computational methods and theoretical modelling has opened up the …

We study the effect of dark matter scalar and vector-mediated interactions on dark matter
admixed neutron stars. In particular, we exploit the two-fluid formalism of Tolman …

Neutron Stars (NSs), among the densest objects in the Universe, are exceptional
laboratories for investigating Dark Matter (DM) properties. Recent theoretical and …